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Cerro Chascon-Runtu Jarita complex

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with base altitudes 4,600–4,900 metres (15,100–16,100 ft). The complex is split into a northern group encompassing Cerro Chascon and three other domes (named Cerro Guichi, Morro Chascoso and Pabelloncita Loma), and a southern group of six domes. Their orientation in northwestward direction is
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Watts, Robert B.; de Silva, Shanaka L.; Jimenez de Rios, Guillermina; Croudace, Ian (10 September 1999). "Effusive eruption of viscous silicic magma triggered and driven by recharge: a case study of the Cerro Chascon-Runtu Jarita Dome Complex in Southwest Bolivia".
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Salisbury, M. J.; Jicha, B. R.; de Silva, S. L.; Singer, B. S.; Jimenez, N. C.; Ort, M. H. (21 December 2010). "40Ar/39Ar chronostratigraphy of Altiplano-Puna volcanic complex ignimbrites reveals the development of a major magmatic province".
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Geochemical analysis led de Silva (1994) to suggest that they may be the latest eruptive cycle of the APVC, either as part of a reactivation or waning of that system. Pastos Grandes is the source of two major ignimbrites, the 8.1
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Cerro Chascon is formed from a cicle of lava flow lobes with a central plug with a diameter of 200 metres (660 ft). Explosive activity occurred before the dome formation and generated a 1 metre (3 ft 3 in) thick
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beneath the dome. The lava dome has a volume of 5 cubic kilometres (1.2 cu mi) with a maximum altitude of 5,190 metres (17,030 ft). Its surface is covered by mounds (20 metres (66 ft) high) of presumably
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Accompanied with little explosive activity on the main dome Cerro Chascon, it contains ten lava domes arranged in a chain. Located in the floor of the Pastos Grandes caldera, these domes were erupted after injection of
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and influenced by local lakewaters. In the southern domes, some time occurred between the formation of the andesitic magmas by mixing and the eruption. Both andesitic and rhyolitic magmas were simultaneously extruded.
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consistent with the regional trends but may also be influenced by the Pastos Grandes caldera structure. The arid climate of the area has impeded erosion in the area, leaving the volcanic complex relatively unaltered.
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de Silva, S. L.; Self, S.; Francis, P. W.; Drake, R. E.; Carlos, Ramirez R. (1994). "Effusive silicic volcanism in the Central Andes: The Chao dacite and other young lavas of the Altiplano-Puna Volcanic Complex".
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Petrology indicates that the andesitic lavas of the southern domes are derived from the more silicic magmas by addition of more mafic andesites. Conversely, the northern dome magmas formed by
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eruptions took place covering an area of 70,000 square kilometres (27,000 sq mi) triggered by the formation of melts deep in the crust and their subsequent rise to the upper crust.
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Sifon and the 5.3 mya Chuhuilla ignimbrite, as well as the 3.1 mya Cerro Juvina ignimbrite shield on the northern caldera flank. The eruption of this complex may have been formed by a
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and central depressions. The much smaller Cerro Guichi (6 metres (20 ft) high and 25 metres (82 ft) long) may be an exposed
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contents ranges from 35% by volume in dacite and 48% by volume of rhyolite. In the northern group these are primarily composed from
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magmas in the deep less than 100,000 years ago. The largest dome has a volume of 5 cubic kilometres (1.2 cu mi).
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this complex is part of the young surface expression of the APVC and may indicate the future location of a caldera.
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Evolution of the Cerro Chascon-Runtu Jarita Complex in Southwest Bolivia: Implications for Silicic Dome Formation
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origin, and are highly viscous with large difference between two magma types. The lava domes are formed from
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caldera, but it may not be part of that caldera complex proper. The lava dome complex is part of the
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components. They contain a rhyolitic core surrounded with andesitic lavas that contains primarily
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named Runtu Jarita whose largest member is named Cerro Chascon. This chain is comparable with the
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when the injection of new magmas led to eruption. The eruptions of Chascon initially were
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in the north. The dacites are crystal rich and some lavas show evidence of magma mixing.
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magmas in the magmatic system. Presumably, the magmas were in the process of forming a
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Morro Chascoso and Pabelloncita Loma are cone shaped domes with blocky slopes with
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The lava domes were erupted between 89,000-94,000 years ago. In Runtu Jarita,
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phenocrysts. Temperatures of 926–1,000 °C (1,699–1,832 °F) for
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origin, with sand trails eroded from the mounds separating them.
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The lava domes are contained within the moat and floor of the
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with the most evolved components being erupted explosively.
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in the United States. Together with other lava domes like
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Index

21°53′02″S 67°54′18″W / 21.88389°S 67.90500°W / -21.88389; -67.90500
lava domes
Pastos Grandes caldera
Altiplano-Puna volcanic complex
mafic
lava domes
Mono-Inyo craters
Cerro Chao
Pastos Grandes
Altiplano-Puna volcanic complex
Miocene
Pleistocene
ignimbrite
mya
dyke
21°53′S 67°54′W / 21.883°S 67.900°W / -21.883; -67.900
22°02′S 67°49′W / 22.033°S 67.817°W / -22.033; -67.817
pumice
rhyolitic
obsidian
diapiric
talus
intrusion
andesitic
lava flow
potassium
calc-alkaline
andesite
dacite
Phenocryst

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